Astronomy and Astrophysics – Astronomy
Scientific paper
Mar 1993
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1993stin...9413483s&link_type=abstract
Presented at the International Gamma-Ray Astrophysics Laboratory Integral Workshop, Les Diablerets, Switzerland, 2-5 Feb. 1993
Astronomy and Astrophysics
Astronomy
Crystals, Diffraction, Gamma Ray Telescopes, Gamma Rays, Laue Method, Lenses, Photons, Positron Annihilation, Positrons, Angular Resolution, Gamma Ray Astronomy, Germanium, Gondolas, Quasars, Radiation Detectors
Scientific paper
We present a new type of gamma-ray telescope featuring a Laue diffraction lens, a detector module with a 3-by-3 germanium array, and a balloon gondola stabilized to 5 arc sec pointing accuracy. The instrument's lens is designed to collect 511 keV photons on its 150 sq cm effective area and focus them onto a small detector having only (approx) 14 cu cm of equivalent volume for background noise. As a result, this telescope overcomes the mass-sensitivity impasse of present detectors in which the collection areas are identical to the detection area. The sensitivity of our instrument is anticipated to be 3 (times) 10-5 ph cm-2 S-1 at 511 keV with an angular resolution of 15 arc sec and an energy resolution of 2 keV. These features will allow the resolve of a possible energetically narrow 511 keV positron annihilation line both energy-wise and spatially within a Galactic Center 'microquasar' as 1El740.7-2942 or GRS1758-258. In addition to the galactic 'microquasars', other prime objectives include Cyg X-1, X-ray binaries, pulsars, and AGNS.
Smither Robert K.
von Ballmoos Peter.
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